Published 1991
| public
Book Section - Chapter
A Subpixel Deconvolution Method for Astronomical Images
- Creators
- Weir, N.
-
Djorgovski, S.
- Others:
- Grandy, W. T., Jr.
- Schick, L. H.
Chicago
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Abstract
We present results from the use of an image deconvolution method for achieving subpixel resolution in certain data regimes. Restorations are performed using a shell which utilizes the Gull-Skilling MEMSYS-3 package. We have performed extensive tests using the method and have determined general limits of its applicability and resolving power. We present results from applying the technique to simulated and real images of sparse and closely crowded astronomical fields. Specific projects involved in this study include a search for close companions to quasars and the structural investigation of star cluster cores.
Additional Information
© 1991 Springer Science+Business Media Dordrecht. We wish to thank Steve Gull for his help and insight in implementing MEMSYS-3. This material is based upon work supported under a National Science Foundation Graduate Fellowship (NW), and in part by the Alfred P. Sloan Foundation (SD).Additional details
- Eprint ID
- 96243
- Resolver ID
- CaltechAUTHORS:20190610-123510979
- NSF Graduate Research Fellowship
- Alfred P. Sloan Foundation
- Created
-
2019-06-10Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- Fundamental Theories of Physics
- Series Volume or Issue Number
- 43